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Rauscher, T, Travaglio, C, Gallino, R, Nishimura, N and Hirschi, R (2014) Production of 92Nb, 92Mo, and 146Sm in the gamma-process in SNIa. In: 13th Symposium on Nuclei in the Cosmos (NIC XIII), Jul 2014, Debrecen, Hungary.

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Abstract

The knowledge of the production of extinct radioactivities like 92Nb and 146Sm by photodisintegration processes in ccSN and SNIa models is essential for interpreting abundances in meteoritic material and for Galactic Chemical Evolution (GCE). The 92Mo/92Nb and 146Sm/144Sm ratios provide constraints for GCE and production sites. We present results for SNIa with emphasis on nuclear uncertainties.

Item Type: Conference or Workshop Item (Paper)
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Natural Sciences > School of Physical and Geographical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 29 Jan 2015 15:17
Last Modified: 29 Sep 2015 10:38
URI: https://eprints.keele.ac.uk/id/eprint/226

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